The NIKA2 Sunyaev–Zeldovich Large Program (LPSZ) observes galaxy clusters with the NIKA2 camera [1]}, [2]}, which is a dual–band millimeter continuum instrument installed at the IRAM 30–meter telescope located at Pico Veleta, Spain. It is capable of mapping the sky simultaneously at \(150 \ \mathrm {GHz}\)  and \(260 \ \mathrm {GHz}\)  using kinetic inductance detectors or KIDs [3]}. The camera has a field of view of \(6.5^{\prime }\)  and a high angular resolution of \(17.6^{\prime \prime }\)  and \(11.1^{\prime \prime }\)  at \(150 \ \mathrm {GHz}\)  and \(260 \ \mathrm {GHz}\) , respectively. The sensitivity at the two respective wavelengths is also high, standing at \( 9 \ \mathrm {and} \ 30 \ \mathrm {mJy \ s^{\frac{1}{2}}}\) , respectively. Details of the performance of the camera can be found in [4]}. The instrument has been proven to be well–designed for mapping the ICM of galaxy clusters and their thermodynamic properties at intermediate to high redshift (see e.g. [5]}, [6]}).
